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Stars in young nearby associations are the only targets allowing giant planetsearches at all separations in the near future, by coupling indirect techniquessuch as radial velocity and deep imaging. These stars are first prioritiestargets for the forthcoming planets imagers on 10-m class telescopes. Youngstars rotate more rapidly and are more active than their older counterparts.Both effects can limit the capability to detect planets using RV. We wish toexplore the planet detection capabilities of a representative sample of starsin close and young associations with radial velocity data and explore thecomplementarity between this technique and direct imaging. We observed 26 suchtargets with spectral types from A to K and ages from

Planets around stars in young nearby associations *** radial Velocity searches: a feasibility study, and first results